A GLIMPSE into the very faint end of the Hβ+[O III]λλ4960,5008 luminosity function at z ∼ 7 – 9 behind Abell S1063

We used the ultra-deep GLIMPSE JWST/NIRCam survey to constrain the faint end of the [O III]+Hβ luminosity function (LF) down to 1039erg s−1 at z ∼ 7 − 9 behind the lensed Hubble Frontier Field galaxy cluster Abell S1063. We applied a spectral energy distribution fitting on a Lyman-break galaxy selec...

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Váldodahkkit:	Korber Damien, Chemerynska Iryna, Furtak Lukas J., Atek Hakim, Endsley Ryan, Schaerer Daniel, Chisholm John, Kokorev Vasily, Saldana-Lopez Alberto, Adamo Angela, Muñoz Julian B., Oesch Pascal A., Meyer Romain, Marques-Chaves Rui, Fujimoto Seiji
Materiálatiipa:	Artigo
Giella:	Inglês
Almmustuhtton:	EDP Sciences 2026-04-01
Ráidu:	Astronomy & Astrophysics
Fáttát:	galaxies: dwarf galaxies: high-redshift galaxies: luminosity function mass function galaxies: photometry galaxies: star formation dark ages reionization first stars
Liŋkkat:	https://www.aanda.org/articles/aa/full_html/2026/04/aa56868-25/aa56868-25.html
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